Gain Notes for Revolution 2682 No JEM-X2 science data for this revolution due to re-allocation of TM packets. This revolution contains a TOO observation of Swift J1727.8-1613, a very strong blackhole source which caused extensive greyfiltering which largely swamped and destroyed the Xe line. At the same time the Sun, approaching Solar Max, was very active during this revolution (low latitude aurorae observed) and this has produced radical gain suppression, below 20 chans/keV which means all the low-level photons (about 5keV and below, depending on the exact value of the detector gain) will have disappeare into the low level discriminator - i.e. filtered out onboard as electronic noise. For this reason the entire revolution will be considered a BTI. Without this solar activity, the TOO observation alone would be the BTI. BTI = 8646.8 to 8649.2 IJD. This data is not suitable for spectra or low energy lightcurves. This is one of the later revolutions in the mission where the calibration sources have become so weak that for the best energy determination an IC Gain History table is needed. These gain history tables are found automatically by OSA, or can be downloaded from the DTU FTP site. All offline gain/energy corrections (including the IC tables) are based on the two Fe calibration sources in JEM-X1, for both units, then corrected iteratively using the instrument background lines (Xe, backed up by Cu and Mo). Latest OSA software (version 10 and higher) automatically cuts out the first Science windows of data from each revolution to ensure that people do not use data from the instrument-settling period. This process can be overruled, but only by experienced users. JEM-X1 rating: Very good outside of the TOO observation, but whole revolution is declared at BTI due to the extreme gain suppression due to solar activity that sends all the low-energy photons into the low-level discriminator to be discarded as electronic noise. JEM-X2: No data - TM packets allocated to SPI and IBIS. CAO 07/09/2023